Search for the gamma-ray spectral lines with the DAMPE and the Fermi-LAT observations
Physical Review D(2023)
摘要
Weakly interacting massive particles, as a major candidate of dark matter
(DM), may directly annihilate or decay into high-energy photons, producing
monochromatic spectral lines in the gamma-ray band. These spectral lines, if
detected, are smoking-gun signatures for the existence of new physics. Using
the 5 years of DAMPE and 13 years of Fermi-LAT data, we search for line-like
signals in the energy range of 3 GeV to 1 TeV from the Galactic halo. Different
regions of interest are considered to accommodate different DM density
profiles. We do not find any significant line structure, and the previously
reported line-like feature at ∼133 GeV is also not detected in our
analysis. Adopting a local DM density of ρ_ local=0.4
GeV cm^-3, we derive 95
velocity-averaged cross-section of ⟨σ v⟩_γγ≲ 4 × 10^-28 cm^3 s^-1 and the decay lifetime of
τ_γν≳ 5 × 10^29 s at 100 GeV, achieving the
strongest constraints to date for the line energies of 6-660 GeV. The
improvement stems from the longer Fermi-LAT data set used and the inclusion of
DAMPE data in the analysis. The simultaneous use of two independent data sets
could also reduce the systematic uncertainty of the search.
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关键词
spectral lines,dampe,gamma-ray,fermi-lat
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